Metastable dark matter from primordial black hole evaporation can produce PeV-EeV neutrinos matching KM3-230213A and IceCube observations while satisfying relic abundance constraints.
Cosmological origin of the km3-230213a event and associated gravitational waves
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PBHs must exceed 10^9 g to affect BBN observables, yielding beta upper limits from 10^{-17} to 10^{-19} for masses 10^9-10^10 g, with public code provided.
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KM3-230213A and IceCube Neutrino Events from Metastable Dark Matter of Primordial Black Hole Origin
Metastable dark matter from primordial black hole evaporation can produce PeV-EeV neutrinos matching KM3-230213A and IceCube observations while satisfying relic abundance constraints.
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Primordial Black Holes Evaporating before Big Bang Nucleosynthesis
PBHs must exceed 10^9 g to affect BBN observables, yielding beta upper limits from 10^{-17} to 10^{-19} for masses 10^9-10^10 g, with public code provided.